Abstract
We investigate the possibility of a future singularity due to accelerating expansion of the Universe in a gravitational theory that comprises the Ricci scalar \(R\) and the Gauss–Bonnet invariant \(\mathcal{G}\), known as \(F(R,\mathcal{G})\) gravity, which can be viewed in the quadratic form. Three models are presented using Hubble parameters to represent a finite and infinite future. The model parameters are analyzed on the basis of their physical and geometrical properties. This study also explores the properties of the modified gravitational theory, and neither a future singularity nor a little or pseudo-rip are posed as threats to the fate of the Universe. We present scalar perturbation approaches to perturbed evolution equations and demonstrate their stability.
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Funding
SVL acknowledges the financial support provided by the University Grants Commission through the Junior Research Fellowship (Ref. no. 191620116597) to carry out the research work. F. Tello-Ortiz thanks the financial support of projects ANT-1956 and SEM 18-02 at the Universidad de Antofagasta, Chile. F. Tello-Ortiz acknowledges the PhD program Doctorado en FAsica mencion en Fisica Matematica de la Universidad de Antofagasta for continuous support and encouragement. BM and SKT acknowledge IUCAA, Pune, India, for support through the visiting associateship programme.
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Lohakare, S.V., Tello-Ortiz, F., Mishra, B. et al. The Fate of the Universe Evolution in the Quadratic Form of Ricci–Gauss–Bonnet Cosmology. Gravit. Cosmol. 29, 443–455 (2023). https://doi.org/10.1134/S0202289323040138
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DOI: https://doi.org/10.1134/S0202289323040138